the xmm-newton cross-calibration campaign
DESCRIPTION
The XMM-Newton cross-calibration campaign. M.G.F. Kirsch, A.M.T. Pollock, B.Chen, M.Smith M.M. Sierra, L. Metcalfe, B. Altieri. EPIC and RGS ratio. menu. objectives schedule methods outcome (so far). objectives. systematic XSA data mining public CCFs and SAS - PowerPoint PPT PresentationTRANSCRIPT
Marcus KirschMarcus Kirsch
Science Operations & Data Systems Division Research & Scientific Support Department
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XMM-NewtonXMM-Newton
EPICEPIC
The XMM-Newton The XMM-Newton cross-calibration campaigncross-calibration campaign
M.G.F. Kirsch, A.M.T. Pollock, M.G.F. Kirsch, A.M.T. Pollock, B.Chen, M.Smith B.Chen, M.Smith
M.M. Sierra, L. Metcalfe, B. Altieri M.M. Sierra, L. Metcalfe, B. Altieri
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
Page 2
XMM-NewtonXMM-Newton
EPICEPICEPIC and RGS ratioEPIC and RGS ratio
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
Page 3
XMM-NewtonXMM-Newton
EPICEPICmenumenu
objectivesobjectives
schedule schedule
methodsmethods
outcome (so far)outcome (so far)
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
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XMM-NewtonXMM-Newton
EPICEPICobjectivesobjectives
systematic XSA data miningsystematic XSA data mining
public CCFs and SAS public CCFs and SAS
2525 targets, 200targets, 200 observations observations
line-rich spectra RGS line-rich spectra RGS EPIC EPIC
continuum spectra EPIC continuum spectra EPIC RGS RGS
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
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XMM-NewtonXMM-Newton
EPICEPICscheduleschedule
2003/05: start of campaign2003/05: start of campaign 2003/07: start of data analysis2003/07: start of data analysis 2003/09: first results2003/09: first results
2003/11: Chandra exchange2003/11: Chandra exchange 2004/05: Green Paper 2004/05: Green Paper 2004/07: White Paper 2004/07: White Paper
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
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XMM-NewtonXMM-Newton
EPICEPICtargets treated targets treated line-rich sources:line-rich sources:
– SNR 1E0102-7219 (8)SNR 1E0102-7219 (8)– AB Dor (8)AB Dor (8)– SNR N132D (14)SNR N132D (14)– Capella (6)Capella (6)
continuum sourcescontinuum sources– PKS2155-304 (9)PKS2155-304 (9)– PKS0558-504 (4)PKS0558-504 (4)– RXJ1856.6-3754 (1)RXJ1856.6-3754 (1)– RXJ0720.4-3125 (6)RXJ0720.4-3125 (6)– RXJ0806.4-4123 (3)RXJ0806.4-4123 (3)
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
Page 7
XMM-NewtonXMM-Newton
EPICEPICmethodsmethods
extractionextraction– pile-up checkpile-up check– flare screeningflare screening– source and background extractionsource and background extraction– response matrix generationresponse matrix generation
modellingmodelling assessmentassessment
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
Page 8
XMM-NewtonXMM-Newton
EPICEPICresults: PKS2155-304results: PKS2155-304
Model: constant Model: constant *wabs *wabs *powerlaw*powerlawwhere constants for where constants for RGS are free RGS are free (0.91,0.89), all (0.91,0.89), all other parameters other parameters are fitted are fitted simultaneouslysimultaneously
up to ± 20% up to ± 20% differences in fluxdifferences in flux
same trend also same trend also observed for observed for PKS0558-504PKS0558-504
Marcus KirschMarcus KirschScience Operations & Data Systems Division
Research & Scientific Support Department
Page 9
XMM-NewtonXMM-Newton
EPICEPICresults: AB Dorresults: AB Dor
Model: Model: constant *wabs constant *wabs *(vmekal+bremss)*(vmekal+bremss)where constants for where constants for RGS are free RGS are free (0.85,0.87), (0.85,0.87), all other parameters all other parameters are fitted are fitted simultaneouslysimultaneously
the spectrum’s many the spectrum’s many lines are not perfectly lines are not perfectly fit but the model is fit but the model is good enough for this good enough for this comparisoncomparison
up to ± 20% up to ± 20% differences in flux differences in flux